Repository logo
  • English
  • Italiano
Log In
Have you forgotten your password?
  1. Home
  2. PRODOTTI RICERCA INAF
  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
  4. 1.01 Articoli in rivista
  5. First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O iii]/H α Emitter at z = 6.11
 

First Peek with JWST/NIRCam Wide-field Slitless Spectroscopy: Serendipitous Discovery of a Strong [O iii]/H α Emitter at z = 6.11

Journal
THE ASTROPHYSICAL JOURNAL LETTERS  
Date Issued
2022
Author(s)
Sun, Fengwu
•
Egami, Eiichi
•
Pirzkal, Nor
•
Rieke, Marcia
•
Boyer, Martha
•
CORRENTI, Matteo  
•
Gennaro, Mario
•
Girard, Julien
•
Greene, Thomas P.
•
Kelly, Doug
•
Koekemoer, Anton M.
•
Leisenring, Jarron
•
Misselt, Karl
•
Nikolov, Nikolay
•
Roellig, Thomas L.
•
Stansberry, John
•
Williams, Christina C.
•
Willmer, Christopher N.A.
DOI
10.3847/2041-8213/ac8938
Abstract
We report the serendipitous discovery of an [O iii] λ λ4959/5007 and Hα line emitter in the Epoch of Reionization (EoR) with the James Webb Space Telescope (JWST) commissioning data taken in the NIRCam wide-field slitless spectroscopy (WFSS) mode. Located 1/455″ away from the flux calibrator P330-E, this galaxy exhibits bright [O iii] λ λ4959/5007 and Hα lines detected at 3.7σ, 9.9σ, and 5.7σ, respectively, with a spectroscopic redshift of z = 6.112 ± 0.001. The total Hβ+[O iii] equivalent width is 664 ± 98 Å (454 ± 78 Å from the [O iii] λ5007 line). This provides direct spectroscopic evidence for the presence of strong rest-frame optical lines (Hβ+[O iii] and Hα) in EoR galaxies as inferred previously from the analyses of the Spitzer/IRAC spectral energy distributions (SEDs). Two spatial and velocity components are identified in this source, possibly indicating that this system is undergoing a major merger, which might have triggered the ongoing starburst with strong nebular emission lines over a timescale of 1/42 Myr, as our SED modeling suggests. The tentative detection of He ii λ4686 line (1.9σ), if real, may indicate the existence of very young and metal-poor star-forming regions with a hard UV radiation field. Finally, this discovery demonstrates the power and readiness of the JWST/NIRCam WFSS mode, and marks the beginning of a new era for extragalactic astronomy, in which EoR galaxies can be routinely discovered via blind slitless spectroscopy through the detection of rest-frame optical emission lines.
Volume
936
Issue
1
Start page
L8
Uri
http://hdl.handle.net/20.500.12386/36472
Url
https://api.elsevier.com/content/abstract/scopus_id/85137691834
https://iopscience.iop.org/article/10.3847/2041-8213/ac8938
Issn Identifier
2041-8205
Rights
open.access
File(s)
Loading...
Thumbnail Image
Name

Sun_2022_ApJL_936_L8.pdf

Description
Pdf editoriale
Size

985.98 KB

Format

Adobe PDF

Checksum (MD5)

c3c789ceb6bcf6bb311b85199beb1c3e

Explore By
  • Communities and Collection
  • Research Outputs
  • Researchers
  • Organizations
  • Projects
Information and guides for authors
  • https://openaccess-info.inaf.it: all about open access in INAF
  • How to enter a product: guides to OA@INAF
  • The INAF Policy on Open Access
  • Downloadable documents and templates

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback